The issue of HD 118508 is a topic that has generated great interest and controversy in recent times. With different approaches and perspectives, HD 118508 has been the subject of debate and research in various areas of knowledge. From its impact on society to its implications at the individual level, HD 118508 has captured the attention of academics, specialists and ordinary people. In this article, we will explore different aspects related to HD 118508, analyzing its relevance and unraveling its possible consequences. Additionally, we will examine how HD 118508 has shaped and will continue to shape the current landscape, offering a comprehensive view of this important topic.
HD 118508 is a suspected variable star in the northern constellation of Boötes. Its apparent magnitude may vary with an amplitude of 0.04, discovered during a search for small-amplitude red variables.[7] It is a red giant about 552 light years away.
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^ abPercy, John R.; Au, Winnie (November 1994), "APT Observations of Small-Amplitude Red Variables", Information Bulletin on Variable Stars, 4114 (4114): 1, Bibcode:1994IBVS.4114....1P
^Gontcharov, G. A. (2017), "VizieR Online Data Catalog: Tycho-2 red giant branch and carbon stars (Gontcharov, 2011)", VizieR On-line Data Catalog, Bibcode:2017yCat..90370769G
^ abcdAnders, F.; Khalatyan, A.; Chiappini, C.; Queiroz, A. B.; Santiago, B. X.; Jordi, C.; Girardi, L.; Brown, A. G. A.; Matijevič, G.; Monari, G.; Cantat-Gaudin, T.; Weiler, M.; Khan, S.; Miglio, A.; Carrillo, I.; Romero-Gómez, M.; Minchev, I.; De Jong, R. S.; Antoja, T.; Ramos, P.; Steinmetz, M.; Enke, H. (2019), "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18", Astronomy and Astrophysics, 628: A94, arXiv:1904.11302, Bibcode:2019A&A...628A..94A, doi:10.1051/0004-6361/201935765, S2CID131780028